Search Results - "M. A. Bykov"
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GEMINGA'S PUZZLING PULSAR WIND NEBULA
Published in The Astrophysical journal (20-01-2017)“…ABSTRACT We report on six new Chandra observations of the Geminga pulsar wind nebula (PWN). The PWN consists of three distinct elongated structures-two 0.2 d…”
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Shocks and Non-thermal Particles in Clusters of Galaxies
Published in Space science reviews (01-02-2019)“…Galaxy clusters grow by gas accretion, mostly from mergers of substructures, which release powerful shock waves into cosmic plasmas and convert a fraction of…”
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Ultrahard spectra of PeV neutrinos from supernovae in compact star clusters
Published in Monthly notices of the Royal Astronomical Society (11-10-2015)“…Starburst regions with multiple powerful winds of young massive stars and supernova remnants are favourable sites for high-energy cosmic ray (CR) acceleration…”
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Observational Signatures of Particle Acceleration in Supernova Remnants
Published in Space science reviews (01-11-2012)“…We evaluate the current status of supernova remnants as the sources of Galactic cosmic rays. We summarize observations of supernova remnants, covering the…”
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Diffusive Shock Acceleration and Magnetic Field Amplification
Published in Space science reviews (01-11-2012)“…Diffusive shock acceleration is the theory of particle acceleration through multiple shock crossings. In order for this process to proceed at a rate that can…”
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Large-Scale Structure Formation: From the First Non-linear Objects to Massive Galaxy Clusters
Published in Space science reviews (01-05-2015)“…The large-scale structure of the Universe formed from initially small perturbations in the cosmic density field, leading to galaxy clusters with up to 10 15 M…”
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Observations of Extended Radio Emission in Clusters
Published in Space science reviews (01-02-2008)“…We review observations of extended regions of radio emission in clusters; these include diffuse emission in ‘relics’, and the large central regions commonly…”
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Cosmic ray current driven turbulence in shocks with efficient particle acceleration: the oblique, long-wavelength mode instability
Published in Monthly notices of the Royal Astronomical Society (01-01-2011)“…In order for diffusive shock acceleration (DSA) to accelerate particles to high energies, the energetic particles must be able to interact with magnetic…”
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Fundamentals of collisionless shocks for astrophysical application, 2. Relativistic shocks
Published in The Astronomy and astrophysics review (01-12-2011)“…In this concise review of the recent developments in relativistic shock theory in the Universe we restrict ourselves to shocks that do not exhibit quantum…”
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Non-Thermal Processes in Cosmological Simulations
Published in Space science reviews (01-02-2008)“…Non-thermal components are key ingredients for understanding clusters of galaxies. In the hierarchical model of structure formation, shocks and large-scale…”
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Editorial to the Topical Collection on Clusters of Galaxies: Physics and Cosmology
Published in Space science reviews (01-04-2019)Get full text
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Cobalt–Samarium Oxide Composite as a Novel High-Performance Catalyst for Partial Oxidation and Dry Reforming of Methane into Synthesis Gas
Published in Petroleum chemistry (01-03-2023)“…The paper describes a novel high-performance catalyst that was developed for partial oxidation of methane (POM) and dry reforming of methane (DRM) into…”
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Novel Samarium Cobaltate/Silicon Carbide Composite Catalyst for Dry Reforming of Methane into Synthesis Gas
Published in Petroleum chemistry (01-05-2023)“…The paper describes a specifically developed novel samarium cobaltate/silicon carbide composite that transforms into a high-performance carbon-resistant…”
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Novel High-Performance Catalysts for Partial Oxidation and Dry Reforming of Methane to Synthesis Gas
Published in Petroleum chemistry (01-05-2022)“…High-performance catalysts for partial oxidation (POM) and dry reforming of methane (DRM) into synthesis gas with a yield of more than 90% have been developed…”
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15
Determination of Computer Code Error by Experimental Results
Published in Physics of atomic nuclei (01-12-2020)“…We determine the computer code error taking into account errors of experiments. Using the statistical simulation methods, we find the error taking into account…”
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A model of polarized X-ray emission from twinkling synchrotron supernova shells
Published in Monthly notices of the Royal Astronomical Society (01-11-2009)“…Synchrotron X-ray emission components were recently detected in many young supernova remnants (SNRs). There is even an emerging class – SN 1006, RX…”
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Simulation of Accelerated Particle Diffusion in Collisionless Shocks with an Admixture of Heavier-than-Hydrogen Ions
Published in Technical physics (2020)“…We report on the results of hybrid simulation of diffusive shock acceleration of ions with different charge-to-mass ratios in quasi-parallel collisionless…”
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Pulsar Wind Nebulae with Bow Shocks: Non-thermal Radiation and Cosmic Ray Leptons
Published in Space science reviews (01-07-2017)“…Pulsars with high spin-down power produce relativistic winds radiating a non-negligible fraction of this power over the whole electromagnetic range from radio…”
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Effect of the Support Nature on Stability of Nickel and Nickel–Cobalt Catalysts for Partial Oxidation and Dry Reforming of Methane to Synthesis Gas
Published in Petroleum chemistry (01-04-2019)“…It has been shown that the nature of the support (MFI zeolite, aluminum–magnesium hydrotalcite, stabilized ceria, neodymia) has a significant effect on the…”
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Inside the core of a young massive star cluster: 3D MHD simulations
Published in Monthly notices of the Royal Astronomical Society (19-10-2022)“…ABSTRACT Young massive star clusters inhabit regions of star formation and play an essential role in the galactic evolution. They are sources of both thermal…”
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